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- W3174443616 abstract "We wish to assess the relationship between the population of planetary nebulae (PNe) and a given parent stellar population from a theoretical point of view. Our results rely on original population synthesis models used to estimate the expected luminosity-specific PN density and account for different evolutionary scenarios and star formation histories, as observed in galaxies in the near Universe. For a complete PN sample, we find that 1 PN/1.5106 L⊙ is a safe (IMF-independent) lower limit to the traced global bolometric luminosity of the parent stellar population. A tentative application to Virgo cluster data allows us to place a lower limit at ~ 7% for the global B luminosity of the cluster provided by “loose” intergalactic stars." @default.
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- W3174443616 date "2006-10-06" @default.
- W3174443616 modified "2023-10-12" @default.
- W3174443616 title "Planetary Nebulae as Tracers of the Intergalactic Stellar Background: A Population Synthesis Theoretical Approach" @default.
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- W3174443616 doi "https://doi.org/10.1007/11604792_54" @default.
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